Saharan dust outbreak over southeastern Spain as detected by sun photometer

被引:101
作者
Lyamani, H [1 ]
Olmo, FJ [1 ]
Alados-Arboledas, L [1 ]
机构
[1] Univ Granada, Fac Ciencias, Dept Fis Aplicada, Granada 18071, Spain
关键词
aerosol properties; sun photometry; Angstrom parameter; Saharan dust;
D O I
10.1016/j.atmosenv.2005.09.011
中图分类号
X [环境科学、安全科学];
学科分类号
08 ; 0830 ;
摘要
continent that permit studying the Saharan dust just entering European continent before its possible mixing with anthropogenic emissions in Europe. Two Saharan dust events that occurred during 30 August-3 September and on 10 September 1998 were observed at an inland location on the outskirts of Granada in southeastern Spain. Detailed analyses including back trajectories and TOMS aerosol index maps showed transport of Saharan dust from the Sahara desert and North Africa to the study area. The dust episodes were associated with marked increases in aerosol optical depth (delta(a)) at all wavelengths examined in this study. Thus delta(a) (500 nm) increased from a value of similar to 0.2 corresponding to normal conditions tip to 0.6 in the first event and up to 0.55 in the second. At the end of these events, the arrival of air masses from the Atlantic caused a sharp decrease in delta(a) (500nm) that reaches values close to those obtained before the event (similar to 0.2). The Angstrom exponent alpha reached a minimum of 0.36 in the first event and 0.37 in the second. The Angstrom exponent alpha and aerosol optical depth values during dust events agree well with those obtained under the same kind of events in AERONET and SKYNET sites, as well as with the results obtained in ACE-2 and ACE-Asia experiments. The aerosol size distributions, retrieved from aerosol optical depth using King's method, demonstrated how the large size fraction of aerosol associated with Saharan dust dominated during these events. When Saharan dust was present, the retrieved aerosol size distributions were bimodal with a well-defined mode centred at a radius of 0.6 mu m, and showed an evident increase in the large particles mode with radii in the range 0.4-2 mu m. The small particle concentration during the two events did not present any marked change, and was similar to those observed on days without Saharan dust. Large particle concentration was higher by a factor of 8 than during normal conditions. (c) 2005 Elsevier Ltd. All rights reserved.
引用
收藏
页码:7276 / 7284
页数:9
相关论文
共 38 条
[1]   Physical characteristics of Saharan dust near the Gulf of Guinea [J].
Afeti, GM ;
Resch, FJ .
ATMOSPHERIC ENVIRONMENT, 2000, 34 (08) :1273-1279
[2]   Aerosol size properties at Armilla, Granada (Spain) [J].
Alados-Arboledas, L ;
Lyamani, H ;
Olmo, FJ .
QUARTERLY JOURNAL OF THE ROYAL METEOROLOGICAL SOCIETY, 2003, 129 (590) :1395-1413
[3]   Sahara mineral dust measurements from TOMS: Comparison to surface observations over the Middle East for the extreme dust storm, March 14-17, 1998 [J].
Alpert, P ;
Ganor, E .
JOURNAL OF GEOPHYSICAL RESEARCH-ATMOSPHERES, 2001, 106 (D16) :18275-18286
[4]   INVERTING HIGH-SPECTRAL-RESOLUTION AEROSOL OPTICAL DEPTH TO DETERMINE THE SIZE DISTRIBUTION OF ATMOSPHERIC AEROSOL [J].
AMATO, U ;
ESPOSITO, F ;
SERIO, C ;
PAVESE, G ;
ROMANO, F .
AEROSOL SCIENCE AND TECHNOLOGY, 1995, 23 (04) :591-602
[5]   Simulation of mineral dust effects on UV radiation levels [J].
Díaz, JP ;
Expósito, FJ ;
Torres, CJ ;
Carreño, V ;
Redondas, A .
JOURNAL OF GEOPHYSICAL RESEARCH-ATMOSPHERES, 2000, 105 (D4) :4979-4991
[6]  
Draxler R.R., 1997, NOAA TECHNICAL MEMOR, P24
[7]  
Dubovik O, 2002, J ATMOS SCI, V59, P590, DOI 10.1175/1520-0469(2002)059<0590:VOAAOP>2.0.CO
[8]  
2
[9]  
Gonzalez-Jorge H., 1996, J ATMOS SCI, V53, P3669
[10]  
HANEL G, 1994, APPL OPTICS, V33, P7187, DOI 10.1364/AO.33.007187